Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters
文献类型：期刊论文
| 作者 | Yang,Yizhao1; Miao,Haitao1,4; Ma,Qinglin1; Liu,Miaoxin1; Sabiu,Cristiano G.3; Forero-Romero,Jaime2; Huang,Yuanzhu1; Lai,Limin1; Qian,Qiyue1; Zheng,Yi1 |
| 刊名 | The Astrophysical Journal
 |
| 出版日期 | 2020-08-27 |
| 卷号 | 900期号:1 |
| 关键词 | Large-scale structure of the universe Cosmological parameters from large-scale structure |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/aba35b |
| 英文摘要 | Abstract We used the mark weighted correlation functions (MCFs), W(s), to study the large-scale structure of the universe. We studied five types of MCFs with the weighting scheme ρα, where ρ is the local density, and α is taken as ?1,??0.5, 0, 0.5, and 1. We found that different MCFs have very different amplitudes and scale dependence. Some of the MCFs exhibit distinctive peaks and valleys that do not exist in the standard correlation functions. Their locations are robust against the redshifts and the background geometry; however, it is unlikely that they can be used as “standard rulers” to probe the cosmic expansion history. Nonetheless, we find that these features may be used to probe parameters related with the structure formation history, such as the values of σ8 and the galaxy bias. Finally, after conducting a comprehensive analysis using the full shapes of the W(s)s and WΔs(μ)s, we found that combining different types of MCFs can significantly improve the cosmological parameter constraints. Compared with using only the standard correlation function, the combinations of MCFs with α?=?0, 0.5, 1 and α?=?0,??1,??0.5, 0.5, 1 can improve the constraints on Ωm and w by ≈30% and 50%, respectively. We find highly significant evidence that MCFs can improve cosmological parameter constraints. |
| 语种 | 英语 |
| WOS记录号 | IOP:0004-637X-900-1-ABA35B |
| 出版者 | The American Astronomical Society |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/61797]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 1.School of Physics and Astronomy, Sun Yat-Sen University, Guangzhou 510297, People's Republic of China 2.Departamento de Física, Universidad de los Andes, Cra. 1 No. 18A-10 Edificio Ip, CP 111711, Bogotá, Colombia 3.Department of Astronomy, Yonsei University, 50 Yonsei-ro, Seodaemun-gu, Seoul, 03722, Republic of Korea 4.Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China |
| 推荐引用方式 GB/T 7714 | Yang,Yizhao,Miao,Haitao,Ma,Qinglin,et al. Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters[J]. The Astrophysical Journal,2020,900(1). |
| APA | Yang,Yizhao.,Miao,Haitao.,Ma,Qinglin.,Liu,Miaoxin.,Sabiu,Cristiano G..,...&Li,Xiao-Dong.(2020).Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters.The Astrophysical Journal,900(1). |
| MLA | Yang,Yizhao,et al."Using the Mark Weighted Correlation Functions to Improve the Constraints on Cosmological Parameters".The Astrophysical Journal 900.1(2020). |
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来源：国家天文台
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